Throughout this work, we assume a \(\Lambda \) CDM cosmology with \(H_0 = 70\,{\rm km\,s^{-1}\,Mpc^{-1}}\) , \(\Omega _\Lambda = 0.70\) , and \(\Omega _{\rm m} = 0.30\) . All magnitudes are given in the AB system [1]} and stellar masses and SFRs are normalized to a [2]} initial mass function (IMF) unless noted otherwise.
